Investigation of the sources of volatile elements in fine-grained regolith on Mars
Introduction: Martian regolith [1] is constituted with different mineral phases of various grain sizes that could originate from local, regional or global sources [2,3]. It corresponds to the ultimate stage of various erosion and weathering processes. Dust (
Authors
- E. Dehouck (ORCID: https://orcid.org/0000-0002-1368-4494)
- P. Pilleri (ORCID: https://orcid.org/0000-0003-4861-0476)
- W. Rapin (ORCID: https://orcid.org/0000-0003-4660-8006)
- G. David (ORCID: https://orcid.org/0000-0002-2719-1586)
- R. C. Wiens (ORCID: https://orcid.org/0000-0002-3409-7344)
- O. Forni (ORCID: https://orcid.org/0000-0001-6772-9689)
- A. Cousin (ORCID: https://orcid.org/0000-0001-7823-7794)
- Olivier Gasnault (ORCID: https://orcid.org/0000-0002-6979-9012)
- P.Y. Meslin
Institutions
- Université Claude Bernard Lyon 1 (FR)
- École Normale Supérieure de Lyon (FR)
- Centre National de la Recherche Scientifique (FR)
- Purdue University West Lafayette (US)
- Observatoire de Paris (FR)
- Laboratoire de Géologie de Lyon : Terre, Planètes et Environnement (FR)
- Institut de Recherche en Astrophysique et Planétologie (FR)
- Université Jean Monnet (FR)
Publication Details
- Published
- 2026-07-02
- DOI
- https://doi.org/10.5194/epsc2026-99
- Primary Topic
- Planetary Science and Exploration
- Type
- article
- Field-Weighted Citation Impact
- 0.00